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20082026
most citedShark: introducing an open source, free and flexible semi-analytic model of galaxy formation

251 citations · 3.1k across the 74 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

astro-ph.CO2018★ 12 cited

nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts

C. Power, P. J. Elahi, C. Welker +11

Galaxy cluster outskirts mark the transition region from the mildly non-linear cosmic web to the highly non-linear, virialised, cluster interior. It is in this transition region th…

astro-ph.GA2018★ 20 cited

Observing Merger Trees in a New Light

Rhys J. J. Poulton, Aaron S. G. Robotham, Chris Power +1

Merger trees harvested from cosmological -body simulations encode the assembly histories of dark matter halos over cosmic time, and are a fundamental component of semi-analytica…

astro-ph.GA2018★ 231 cited

The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

Weiguang Cui, Alexander Knebe, Gustavo Yepes +34

We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…

astro-ph.CO2018★ 12 cited

Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe

Eromanga Adermann, Pascal J Elahi, Geraint F Lewis +1

We compare the evolution of voids formed under the standard cosmological model and two alternative cosmological models. The two models are a quintessence model (CDM) and a Coupl…

astro-ph.GA2018★ 251 cited

Shark: introducing an open source, free and flexible semi-analytic model of galaxy formation

Claudia del P. Lagos, Rodrigo J. Tobar, Aaron S. G. Robotham +4

We present a new, open source, free semi-analytic model (SAM) of galaxy formation, Shark, designed to be highly flexible and modular, allowing easy exploration of different physica…

astro-ph.GA2018★ 58 cited

Introducing a new, robust galaxy finder algorithm for simulations

Rodrigo Cañas, Pascal J. Elahi, Charlotte Welker +4

Identifying galaxies in hydrodynamical simulations is a difficult task, particularly in regions of high density such as galaxy groups and clusters. We present a new scale-free shap…